Rotationally-perturbed orbital elements of close binary systems

Details Rotationally-perturbed orbital elements of close binary systems Rotationally-perturbed orbital elements of close binary systems

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.136..211z&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 136, no. 2, Aug. 1987, p. 211-219.

Statistics

Computation

Binary Stars, Orbital Elements, Computational Astrophysics, Perturbation, Rotation, Secular Variations

Scientific paper

The aim of this investigation is to present the secular and periodic perturbations of the six orbital elements of a close binary system due to rotational distortion. The authors consider very small inclinations ι of the orbital plane of the system, whereas the eccentricity of the orbit may assume any value between 0 < e < 1. The final formulae for the various elements have been expressed by means of the unperturbed true anomaly measured from the ascending node.

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